SDO HMI 2011-10-14 04:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 36.82 | 174.21 | 26.90 | 127.07 | -14.90 | 119.10 | 42.75 | 243.30 | 0.7363 | 218.4 | 205.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.52 | 0.00 | 0.39 | -13.86 | 121.26 | 44.91 | 245.69 | 0.7545 | 517.0 | 453.0 | |
| 0.00 | 2.54 | 0.00 | 1.88 | -13.78 | 120.63 | 44.29 | 245.49 | 0.7476 | 570.0 | 541.0 | |
| 0.00 | 1.22 | 0.00 | 0.90 | -13.43 | 120.21 | 43.86 | 245.73 | 0.7416 | 624.0 | 518.1 | |
| 2.27 | 130.06 | 1.67 | 95.88 | -14.04 | 119.88 | 43.53 | 244.80 | 0.7408 | 716.4 | 352.0 | |
| 1.49 | 1.66 | 1.13 | 1.26 | -16.97 | 120.58 | 44.23 | 241.56 | 0.7611 | 448.6 | 342.3 | |
| 25.45 | -4.00 | 18.79 | -4.00 | -14.68 | 119.91 | 43.56 | 244.02 | 0.7439 | 945.2 | 999999 | |
| 2.80 | 8.05 | 2.08 | 5.98 | -17.61 | 118.87 | 42.52 | 239.86 | 0.7472 | -456.7 | 184.9 | |
| 0.00 | 0.70 | 0.00 | 0.51 | -17.31 | 118.31 | 41.97 | 239.92 | 0.7401 | -244.0 | -226.8 | |
| 0.00 | 1.22 | 0.00 | 0.86 | -14.67 | 116.77 | 40.43 | 242.37 | 0.7104 | -547.0 | -441.9 | |
| 0.00 | 1.22 | 0.00 | 0.86 | -14.32 | 116.69 | 40.35 | 242.78 | 0.7078 | -564.0 | -431.6 | |
| 0.00 | 2.45 | 0.00 | 1.72 | -15.00 | 116.52 | 40.18 | 241.80 | 0.7094 | -582.0 | -517.5 | |
| 0.00 | 1.22 | 0.00 | 0.84 | -14.35 | 115.77 | 39.43 | 242.21 | 0.6978 | -697.0 | -541.4 | |
| 0.00 | 0.96 | 0.00 | 0.66 | -14.53 | 115.69 | 39.35 | 241.92 | 0.6979 | -633.0 | -555.2 | |
| 0.00 | 0.44 | 0.00 | 0.30 | -15.18 | 115.83 | 39.49 | 241.17 | 0.7029 | -637.0 | -547.8 | |
| 4.37 | 4.99 | 2.93 | 3.34 | -12.93 | 114.43 | 38.08 | 243.31 | 0.6751 | 792.5 | 619.4 | |
| 0.00 | 1.22 | 0.00 | 0.85 | -16.48 | 115.13 | 38.78 | 239.08 | 0.7025 | -620.0 | -490.4 | |
| 0.00 | 1.31 | 0.00 | 0.91 | -16.80 | 115.09 | 38.74 | 238.65 | 0.7039 | -413.0 | -323.8 | |
| 0.00 | 1.84 | 0.00 | 1.27 | -16.04 | 114.87 | 38.52 | 239.47 | 0.6972 | -607.0 | -548.0 | |
| 0.44 | 1.84 | 0.30 | 1.27 | -16.33 | 114.90 | 38.55 | 239.12 | 0.6992 | -768.6 | -644.6 | |
| 0.00 | 0.87 | 0.00 | 0.59 | -14.63 | 114.24 | 37.90 | 240.92 | 0.6824 | -508.0 | -365.3 | |
| 0.00 | 3.76 | 0.00 | 2.60 | -16.67 | 114.66 | 38.31 | 238.54 | 0.6986 | -624.0 | -495.3 | |
| 0.00 | 1.40 | 0.00 | 0.96 | -16.34 | 114.50 | 38.15 | 238.86 | 0.6949 | -849.0 | -739.2 | |
| 0.00 | 1.75 | 0.00 | 1.21 | -16.96 | 114.61 | 38.26 | 238.14 | 0.6997 | -596.0 | -432.0 | |
| 0.00 | 0.96 | 0.00 | 0.66 | -16.96 | 114.21 | 37.86 | 237.87 | 0.6955 | -552.0 | -482.0 | |
| 0.00 | 0.61 | 0.00 | 0.42 | -16.14 | 113.98 | 37.63 | 238.78 | 0.6882 | -748.0 | -668.4 | |
| 0.00 | 0.61 | 0.00 | 0.42 | -16.44 | 114.05 | 37.70 | 238.44 | 0.6907 | -663.0 | -616.1 | |
| 0.00 | 0.79 | 0.00 | 0.53 | -15.76 | 113.07 | 36.73 | 238.67 | 0.6761 | -785.0 | -612.4 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |